User:Kepler-1229b/sandbox/jul72195
| Solar eclipse of July 7, 2195 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Partial |
| Gamma | 1.5095 |
| Magnitude | 0.0353 |
| Maximum eclipse | |
| Coordinates | 64°36′N 98°30′E / 64.6°N 98.5°E |
| Times (UTC) | |
| Greatest eclipse | 15:41:21 |
| References | |
| Saros | 120 (71 of 71) |
| Catalog # (SE5000) | 9956 |
A partial solar eclipse will occur on July 7, 2195. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. This will be the 71st and final event of Solar Saros 120.[1]
Visibility
[edit]The eclipse occurs entirely over Russia.
Related eclipses
[edit]Solar eclipses of 2195 to 2199
[edit]- Saros 120: Solar eclipse of July 7, 2195 P
- Saros 125: Solar eclipse of December 31, 2195 P
- Saros 130: Solar eclipse of June 26, 2196 T
- Saros 135: Solar eclipse of December 19, 2196 A
- Saros 140: Solar eclipse of June 15, 2197 A
- Saros 145: Solar eclipse of December 9, 2197 T
- Saros 150: Solar eclipse of June 4, 2198 A
- Saros 155: Solar eclipse of November 28, 2198 T
- Saros 160: Solar eclipse of May 24, 2199 P
- Saros 165: Solar eclipse of November 18, 2199 P
Saros 120
[edit]This eclipse is a part of Saros series 120, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 27, 933 AD. It contains annular eclipses from August 11, 1059 through April 26, 1492; hybrid eclipses from May 8, 1510 through June 8, 1564; and total eclipses from June 20, 1582 through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of annularity was produced by member 11 at 6 minutes, 24 seconds on September 11, 1113, and the longest duration of totality was produced by member 60 at 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occur at the Moon’s descending node of orbit.[2]
| Series members 50–71 occur between 1801 and 2195: | ||
|---|---|---|
| 50 | 51 | 52 |
 November 19, 1816 |
 November 30, 1834 |
 December 11, 1852 |
| 53 | 54 | 55 |
 December 22, 1870 |
 January 1, 1889 |
 January 14, 1907 |
| 56 | 57 | 58 |
 January 24, 1925 |
 February 4, 1943 |
 February 15, 1961 |
| 59 | 60 | 61 |
 February 26, 1979 |
 March 9, 1997 |
 March 20, 2015 |
| 62 | 63 | 64 |
 March 30, 2033 |
 April 11, 2051 |
 April 21, 2069 |
| 65 | 66 | 67 |
 May 2, 2087 |
 May 14, 2105 |
 May 25, 2123 |
| 68 | 69 | 70 |
 June 4, 2141 |
 June 16, 2159 |
 June 26, 2177 |
| 71 | ||
 July 7, 2195 | ||
References
[edit]
- ^ "Saros Series Catalog of Solar Eclipses - Solar Saros 120". eclipse.gsfc/nasa.gov. NASA. 26 September 2009. Retrieved 2 June 2019.
- ^ "NASA - Catalog of Solar Eclipses of Saros 120". eclipse.gsfc.nasa.gov.
.jpg)
